Multiplicity (statistical mechanics) explained

In statistical mechanics, multiplicity (also called statistical weight) refers to the number of microstates corresponding to a particular macrostate of a thermodynamic system.[1] Commonly denoted

\Omega

, it is related to the configuration entropy of an isolated system[2] via Boltzmann's entropy formulaS = k_\text \log \Omega,where

S

is the entropy and

kB

is the Boltzmann constant.

Example: the two-state paramagnet

A simplified model of the two-state paramagnet provides an example of the process of calculating the multiplicity of particular macrostate.[1] This model consists of a system of microscopic dipoles which may either be aligned or anti-aligned with an externally applied magnetic field . Let

N\uparrow

represent the number of dipoles that are aligned with the external field and

N\downarrow

represent the number of anti-aligned dipoles. The energy of a single aligned dipole is

U\uparrow=-\muB,

while the energy of an anti-aligned dipole is

U\downarrow=\muB;

thus the overall energy of the system isU = (N_\downarrow-N_\uparrow)\mu B.

The goal is to determine the multiplicity as a function of ; from there, the entropy and other thermodynamic properties of the system can be determined. However, it is useful as an intermediate step to calculate multiplicity as a function of

N\uparrow

and

N\downarrow.

This approach shows that the number of available macrostates is . For example, in a very small system with dipoles, there are three macrostates, corresponding to

N\uparrow=0,1,2.

Since the

N\uparrow=0

and

N\uparrow=2

macrostates require both dipoles to be either anti-aligned or aligned, respectively, the multiplicity of either of these states is 1. However, in the

N\uparrow=1,

either dipole can be chosen for the aligned dipole, so the multiplicity is 2. In the general case, the multiplicity of a state, or the number of microstates, with

N\uparrow

aligned dipoles follows from combinatorics, resulting in\Omega = \frac = \frac,where the second step follows from the fact that

N\uparrow+N\downarrow=N.

Since

N\uparrow-N\downarrow=-\tfrac{U}{\muB},

the energy can be related to

N\uparrow

and

N\downarrow

as follows:\beginN_\uparrow &= \frac - \frac\\[4pt]N_\downarrow &= \frac + \frac.\end

Thus the final expression for multiplicity as a function of internal energy is\Omega = \frac.

This can be used to calculate entropy in accordance with Boltzmann's entropy formula; from there one can calculate other useful properties such as temperature and heat capacity.

Notes and References

  1. Book: Schroeder . Daniel V. . An Introduction to Thermal Physics . 1999 . Pearson . 9780201380279 . First.
  2. Book: Atkins, Peter. Julio de Paula. 2002. Physical Chemistry. 7th. Oxford University Press.